Statistical errors and systematic biases in the calibration of the convective core overshooting with eclipsing binaries - A case study: TZ Fornacis

Free Access

Fig. 3

Open with DEXTER Download original image

Left: as in left panel of Fig. 1, but assuming an error of 100 K on the secondary effective temperature. Right: as in the left panel of Fig. 1, but halving the errors on the radii. The two panels were obtained by relying on the FRANEC grid of stellar models.

This figure is made of several images, please see below:

Open with DEXTER

Download original image

Open with DEXTER

Download original image

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.